Orbiting Vehicle 1-10 (also known as OV1-10), launched 11 December 1966 along with
OV1-9, was the tenth (seventh successful) satellite in the OV1 series of the United States Air Force's
Orbiting Vehicle
Orbiting Vehicle or OV, originally designated SATAR (SATellite - Atmospheric Research), comprised five different series of standardized American satellites operated by the US Air Force, launched between 1965 and 1971. Forty seven satellites w ...
program. Designed to observe atmospheric
airglow
Airglow is a faint emission of light by a planetary atmosphere. In the case of Earth's atmosphere, this optical phenomenon causes the night sky never to be completely dark, even after the effects of starlight and diffuse sky radiation, diffuse ...
,
X-ray
An X-ray (also known in many languages as Röntgen radiation) is a form of high-energy electromagnetic radiation with a wavelength shorter than those of ultraviolet rays and longer than those of gamma rays. Roughly, X-rays have a wavelength ran ...
and
cosmic radiation
Cosmic rays or astroparticles are high-energy particles or clusters of particles (primarily represented by protons or atomic nuclei) that move through space at nearly the speed of light. They originate from the Sun, from outside of the Sol ...
, OV1-10 returned significant data on the Sun as well as on geophysical phenomena in
Earth's magnetic field
Earth's magnetic field, also known as the geomagnetic field, is the magnetic field that extends from structure of Earth, Earth's interior out into space, where it interacts with the solar wind, a stream of charged particles emanating from ...
. OV1-10 reentered Earth's atmosphere on 30 November 2002.
History
The Orbiting Vehicle satellite program arose from a US Air Force initiative, begun in the early 1960s, to reduce the expense of space research. Through this initiative, satellites would be standardized to improve reliability and cost-efficiency, and where possible, they would fly on test vehicles or be piggybacked with other satellites. In 1961, the Air Force Office of Aerospace Research (OAR) created the Aerospace Research Support Program (ARSP) to request satellite research proposals and choose mission experiments. The USAF Space and Missiles Organization created their own analog of the ARSP called the Space Experiments Support Program (SESP), which sponsored a greater proportion of technological experiments than the ARSP.
Five distinct OV series of standardized satellites were developed under the auspices of these agencies.
The OV1 series was an evolution of the 2.7 m "Scientific Passenger Pods" (SPP), which, starting on 2 October 1961, rode piggyback on suborbital Atlas missile tests and conducted scientific experiments during their short time in space. General Dynamics received a $2 million contract on 13 September 1963 to build a new version of the SPP (called the Atlas Retained Structure (ARS)) that would carry a self-orbiting satellite. Once the Atlas missile and ARS reached apogee, the satellite inside would be deployed and thrust itself into orbit. In addition to the orbital SPP, General Dynamics would create six of these satellites, each to be long with a diameter of , able to carry a payload into a circular orbit.
Dubbed "Satellite for Aerospace Research" (SATAR), the series of satellites was originally to be launched from the
Eastern Test Range
The Eastern Range (ER) is an American rocket range (Spaceport) that supports missile and rocket launches from the two major launch heads located at Cape Canaveral Space Force Station and the Kennedy Space Center (KSC), Florida. The range ha ...
on Atlas missions testing experimental Advanced Ballistic Re-Entry System (ABRES) nosecones. However, in 1964, the Air Force transferred ABRES launches to the
Western Test Range
The Western Range (WR) is the space launch range that supports the rocket launch site, major launch head at Vandenberg Space Force Base. Managed by the Space Launch Delta 30, the WR extends from the West Coast of the United States to 90° ea ...
causing a year's delay for the program. Moreover, because WTR launches would be into polar orbit as opposed to the low-inclination orbits typical of ETR launches, less mass could be lofted into orbit using the same thrust, and the mass of the SATAR satellites had to be reduced.
The OV1 program was managed by Lt. Col. Clyde Northcott, Jr.
Prior to the dual launch of OV1-9 and OV1-10, there had been eight satellites in the OV1 series, the first launched January 21, 1965. All launches had been on Atlas missiles except for
OV1-6, which was programmed for launch out of sequence (after the 14 July 1966 launch of
OV1-7 and
OV1-8[) so that it could be carried on the ]Titan IIIC
The Titan IIIC was an expendable launch system used by the United States Air Force from 1965 until 1982. It was the first Titan (rocket family), Titan booster to feature large solid rocket motors and was planned to be used as a launcher for the D ...
tasked for the Manned Orbiting Laboratory test flight.
Spacecraft design
OV1-10 was, like the rest of the OV1 satellite series, long and in diameter, consisting of a cylindrical experiment housing capped with flattened cones on both ends. It included 5000 flat-faceted solar cells producing 22 watt
The watt (symbol: W) is the unit of Power (physics), power or radiant flux in the International System of Units (SI), equal to 1 joule per second or 1 kg⋅m2⋅s−3. It is used to quantification (science), quantify the rate of Work ...
s of power. Two antennas for transmitting telemetry and receiving commands extended from the sides of the spacecraft. 12 helium-pressurized hydrogen peroxide
Hydrogen peroxide is a chemical compound with the formula . In its pure form, it is a very pale blue liquid that is slightly more viscosity, viscous than Properties of water, water. It is used as an oxidizer, bleaching agent, and antiseptic, usua ...
thrusters provided attitude control. OV1-10 used 6 distinctive extendible booms with masses at the ends for gravity-gradient stabilization
Gravity-gradient stabilization or tidal stabilization is a passive method of stabilizing artificial satellites or space tethers in a fixed orientation using only the mass distribution of the orbited body and the gravitational field. The main adv ...
, two extending in opposite directions for each of yaw, pitch and roll. The longer yaw axis booms, each measuring , were also used to house experiments. The spacecraft was not able to achieve yaw stability, turning 180 degrees upside down on several occasions.
OV1-10 weighed, with its attached Altair booster, .[
]
Experiments
The OV1-10 science package comprised eight experiments. A number of photometer
A photometer is an instrument that measures the strength of electromagnetic radiation in the range from ultraviolet to infrared and including the visible spectrum. Most photometers convert light into an electric current using a photoresistor, ...
s and a Geiger–Müller tube
The Geiger–Müller tube or G–M tube is the sensing element of the Geiger counter instrument used for the detection of ionizing radiation. It is named after Hans Geiger, who invented the principle in 1908, and Walther Müller, who collaborate ...
detected day and nighttime atmospheric airglow
Airglow is a faint emission of light by a planetary atmosphere. In the case of Earth's atmosphere, this optical phenomenon causes the night sky never to be completely dark, even after the effects of starlight and diffuse sky radiation, diffuse ...
. OV1-10 carried a cosmic ray
Cosmic rays or astroparticles are high-energy particles or clusters of particles (primarily represented by protons or atomic nuclei) that move through space at nearly the speed of light. They originate from the Sun, from outside of the ...
telescope and a Sun-pointed X-ray spectrometer
A spectrometer () is a scientific instrument used to separate and measure Spectrum, spectral components of a physical phenomenon. Spectrometer is a broad term often used to describe instruments that measure a continuous variable of a phenomeno ...
for the evaluation of non-terrestrial radiation, complementing OV1-9's experiment package, which was focused on the long term measurement of orbital radiation and its threat to living organisms. Two NASA
The National Aeronautics and Space Administration (NASA ) is an independent agencies of the United States government, independent agency of the federal government of the United States, US federal government responsible for the United States ...
experiments, a magnetometer
A magnetometer is a device that measures magnetic field or magnetic dipole moment. Different types of magnetometers measure the direction, strength, or relative change of a magnetic field at a particular location. A compass is one such device, ...
and an electric field measuring voltmeter
A voltmeter is an instrument used for measuring electric potential difference between two points in an electric circuit. It is connected in parallel. It usually has a high resistance so that it takes negligible current from the circuit.
A ...
housed in two booms used for gravity-gradient stabilization
Gravity-gradient stabilization or tidal stabilization is a passive method of stabilizing artificial satellites or space tethers in a fixed orientation using only the mass distribution of the orbited body and the gravitational field. The main adv ...
, completed the experiment package.
Mission
Launched from Vandenberg's 576-B-3 launch pad on 11 Dec 1966 at 21:09:57 UTC via Atlas D rocket,[ OV1-10 and the co-launched OV1-9 were the first satellites in the OV1 series to be launched into nearly ]polar orbit
A polar orbit is one in which a satellite passes above or nearly above both poles of the body being orbited (usually a planet such as the Earth, but possibly another body such as the Moon or Sun) on each revolution. It has an inclination of abo ...
s as opposed to 144° retrograde orbit
Retrograde motion in astronomy is, in general, orbital or rotational motion of an object in the direction opposite the rotation of its primary, that is, the central object (right figure). It may also describe other motions such as precession or ...
s. The satellite's track, nearly perpendicular to the equator, meant that it followed a meridian
Meridian or a meridian line (from Latin ''meridies'' via Old French ''meridiane'', meaning “midday”) may refer to
Science
* Meridian (astronomy), imaginary circle in a plane perpendicular to the planes of the celestial equator and horizon
* ...
of nearly constant local time, drifting with respect to the ground about one hour per month.[ The "Vertistat" stabilization system, first installed on the failed OV1-7,] did not consistently work to keep the satellite stably oriented. OV1-10 sometimes flipped upside-down, and it was given to occasional rapid yaw (spinning around its center of mass) motions. This data was useful in illustrating ways to improve future gravity-gradient systems.
OV1-10's X-ray spectrometer returned the most comprehensive set of solar X-ray observations to date. These data were enabled scientists to determine the relative density of neon to magnesium in the solar corona through direct observation rather than using complicated mathematical models. The ratio of neon to magnesium was found to be 1.47 to 1 (+/- .38). OV1-10's airglow experiments also returned observations of Stable Auroral Red (SAR) arcs, which occur during geomagnetic storms, during an event that took place 15–17 February 1967.
Legacy and status
OV1-10 reentered Earth's atmosphere on 30 November 2002. The OV1 program ultimately comprised 22 missions, the last flying on 19 September 1971. As of 26 December 2021, OV1-9 is still in orbit, and its position can be tracked on-line.
References
{{Orbital launches in 1966
Spacecraft launched in 1966
Military satellites
Earth imaging satellites